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自旋轨道耦合量子线中磁性杂质间的修正交换相互作用。

Modified exchange interaction between magnetic impurities in spin-orbit coupled quantum wires.

作者信息

Silva Joelson F, Vernek E

机构信息

Instituto de Física, Universidade Federal de Uberlândia, Uberlândia, Minas Gerais 38400-902, Brazil.

出版信息

J Phys Condens Matter. 2019 Apr 3;31(13):135802. doi: 10.1088/1361-648X/ab0076. Epub 2019 Jan 21.

Abstract

Indirect exchange interaction between magnetic impurities in one dimensional systems is a matter of long discussions since Kittel has established that in the asymptotic limit it decays as the inverse of distance x between the impurities. In this work we investigate this problem in a quantum wire with Rashba spin-orbit coupling (SOC). By employing a second order perturbation theory we find that one additional oscillatory term appears in each of the Ruderman-Kittel-Kasuya-Yosida (RKKY), the Dzaloshinkii-Moryia and the Ising couplings. Remarkably, these extra terms resulting from the spin precession of the conduction electrons induced by the SOC do not decay as in the usual RKKY interaction. We show that these extra oscillations arise from the finite momenta band splitting induced by the spin-orbit coupling that modifies the spin-flip scatterings occurring at the Fermi energy. Our findings open up a new perspective in the long-distance magnetic interactions in solid state systems.

摘要

自基特尔确定在渐近极限下,一维系统中磁性杂质之间的间接交换相互作用随杂质间距离(x)的倒数衰减以来,这一问题一直备受讨论。在这项工作中,我们研究了具有 Rashba 自旋轨道耦合(SOC)的量子线中的这个问题。通过采用二阶微扰理论,我们发现,在鲁德曼 - 基特尔 - 卡苏亚 - 吉田(RKKY)、德扎洛欣斯基 - 莫利亚和伊辛耦合中,每一种耦合都出现了一个额外的振荡项。值得注意的是,由 SOC 诱导的传导电子自旋进动产生的这些额外项,并不像通常的 RKKY 相互作用那样衰减。我们表明,这些额外的振荡源于自旋轨道耦合引起的有限动量能带分裂,它改变了在费米能级处发生的自旋翻转散射。我们的发现为固态系统中的长程磁相互作用开辟了一个新的视角。

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